activity
20062019
most citedThe s Process: Nuclear Physics, Stellar Models, Observations

830 citations · 3.2k across the 32 of their papers we have counts for

collaborators

33 papers

astro-ph.GA2019★ 19 cited

Enrichment of the Galactic disc with neutron capture elements: Sr

T. Mishenina, M. Pignatari, T. Gorbaneva +4

The enrichment history of heavy neutron-capture elements in the Milky Way disc provides fundamental information about the chemical evolution of our Galaxy and about the stellar sou…

astro-ph.SR2018★ 35 cited

New constraints on the major neutron source in low-mass AGB stars

Nan Liu, Roberto Gallino, Sergio Cristallo +4

We compare updated Torino postprocessing asymptotic giant branch (AGB) nucleosynthesis model calculations with isotopic compositions of mainstream SiC dust grains from low-mass AGB…

astro-ph.SR2017★ 32 cited

Observing the metal-poor solar neighbourhood: a comparison of galactic chemical evolution predictions

T. Mishenina, M. Pignatari, B. Cot'e +14

Atmospheric parameters and chemical compositions for ten stars with metallicities in the region of -2.2< [Fe/H] <-0.6 were precisely determined using high resolution, high signal t…

nucl-ex2017★ 9 cited

Stellar () cross section of Na

E. Uberseder, M. Heil, F. Käppeler +5

The cross section of the Na()Na reaction has been measured via the activation method at the Karlsruhe 3.7 MV Van de Graaff accelerator. NaCl samples were expose…

astro-ph.SR2017★ 62 cited

Galactic Chemical Evolution: the Impact of the 13C-pocket Structure on the s-process Distribution

S. Bisterzo, C. Travaglio, M. Wiescher +2

The solar s-process abundances have been analyzed in the framework of a Galactic Chemical Evolution (GCE) model. The aim of this work is to implement the study by Bisterzo et al. (…

astro-ph.GA2016★ 33 cited

Mass and Metallicity Requirement in Stellar Models for Galactic Chemical Evolution Applications

Benoit Côté, Christopher West, Alexander Heger +5

We used a one-zone chemical evolution model to address the question of how many masses and metallicities are required in grids of massive stellar models in order to ensure reliable…